The first gravitational wave (GW), emerging from the collision of two black holes,
which shook the optical systems of the GW observatories [1]} can be considered the trigger of a new era in precision astronomy and cosmology. Since then the LIGO-Virgo-KAGRA collaboration detected already 90 GW events [2]} and the worldwide network of ground-based [3]}, [4]}, [5]}, [6]}, [7]}, [8]} as well as space based GW detectors [9]} continues to grow, granting access to an ever broader frequency band and higher sensitivity.
